Zobrazeno 1 - 9
of 9
pro vyhledávání: '"M S Kirsanova"'
Expansion of wind-blown bubbles or HII regions lead to formation of shocks in the interstellar medium, which compress surrounding gas into dense layers. We made spatially and velocity-resolved observations of the RCW~120 PDR and nearby molecular gas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f3dc48a858ad929c25311127588cf252
http://arxiv.org/abs/2212.08702
http://arxiv.org/abs/2212.08702
We study evolution of hydrogenated amorphous carbon (HAC) grains under harsh UV radiation in photo-dissociation regions (PDRs) near young massive stars. Our aim is to evaluate the impact of the HAC grains on formation of observed small hydrocarbons:
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f107a1d34e826a478c422877487db26
http://arxiv.org/abs/2212.04993
http://arxiv.org/abs/2212.04993
We present observations of ammonia emission lines toward the interstellar filament WB~673 hosting the dense clumps WB~673, WB~668, S233-IR and G173.57+2.43. LTE analysis of the lines allows us to estimate gas kinetic temperature ($\lesssim$ 30~K in a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8cbefdb4f9e9f19917219d0c6e9dbb20
Autor:
M. S. Kirsanova, O. L. Ryabukhina
Publikováno v:
Астрономия и исследование космического пространства: Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой.
We study the molecular filament WB 673 which is located at a distance of 1.8 kpc in the giant molecular cloud G174 + 2.5. Observations of ammonia radiolines NH3 (1,1), (2,2) and (3,3) were carried out in 2019 at the Effelsberg observatory (Germany).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3f7436f38b4456e7dac1c1d0591f927e
https://doi.org/10.15826/b978-5-7996-3229-8.43
https://doi.org/10.15826/b978-5-7996-3229-8.43
Publikováno v:
Астрономия и исследование космического пространства: Всероссийская с международным участием научная конференция студентов и молодых ученых, посвященная памяти Полины Евгеньевны Захаровой.
This research is focusing on studying of physical parameters in the S254—S258 star-formation complex. The following parameters were derived: column densities, clump masses, and highdensity tracers optical depth, including CS and HCO+ molecules. Dif
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8ee68ad17e13e369a7f538ab61b08828
https://doi.org/10.15826/b978-5-7996-3229-8.39
https://doi.org/10.15826/b978-5-7996-3229-8.39
Autor:
M. S. Kirsanova, O. L. Ryabukhina
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::3f7263710e4d4901fe0a3656d2fef4f4
https://doi.org/10.15826/b978-5-7996-2935-9.70
https://doi.org/10.15826/b978-5-7996-2935-9.70
Autor:
M. S. Kirsanova, A. F. Punanova
Publikováno v:
Proceedings of the 48-th International student's conferences "Physics of Space".
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::8bf74f13ade52531a85ef71a3cfc1d2e
https://doi.org/10.15826/b978-5-7996-2935-9.54
https://doi.org/10.15826/b978-5-7996-2935-9.54
Publikováno v:
UV Astronomy 2011 ISBN: 9789400725720
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::436989c998f6cc3290c8740e2516a526
https://doi.org/10.1007/978-94-007-2573-7_5
https://doi.org/10.1007/978-94-007-2573-7_5
Autor:
L. D. Anderson, Z. Makai, M. Luisi, M. Andersen, D. Russeil, M. R. Samal, N. Schneider, P. Tremblin, A. Zavagno, M. S. Kirsanova, V. Ossenkopf-Okada, A. M. Sobolev
Publikováno v:
Astrophysical Journal; 9/1/2019, Vol. 882 Issue 1, p1-1, 1p